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2006MNRAS.368.1773P - Mon. Not. R. Astron. Soc., 368, 1773-1786 (2006/June-1)
Further 2MASS mapping of hot dust in planetary nebulae.
PHILLIPS J.P. and RAMOS-LARIOS G.
Abstract (from CDS):
Finally, it is noted that whilst the core of M 2-2 appears to show hot grain emission, this is less the case for its more extended envelope. The situation may, in this case, be similar to that of NGC 2346, in which much of the emission is located within an unresolved nucleus. Similarly, it is noted that in addition to hot dust and gas thermal continua, the emission in the interior of NGC 40 may be enhanced through rotational-vibrational transitions of H2, and/or the 2p3P0-2s3S transition of Hei.
Abstract Copyright: 2006 The Authors. Journal compilation © 2006 RAS
Journal keyword(s): ISM: jets and outflows - planetary nebulae: general
Simbad objects: 26
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